脱靶量估算和广义比例导引

本文提出一种适于真比例导引系统估计脱靶量的方法，依据这种方法，只要知道制导－控制时间延迟、拦截器的目标的相对运动速度等，就可以估计出脱靶量的大小。本文还就减小脱靶量而有采用广义比例导引的前景进行了探讨。     

卫星捕获太阳的新方法

对卫星入轨后捕获太阳的方法进行了研究 ,并对一种有效的控制规律进行了分析计算 ,最后对卫星的运动过程进行了仿真验证     

准直式地球模拟器锗准直透镜光学系统的设计

从视场设计出发 ,分析了锗基片的厚度和光学材料吸收特性对光学设计的影响 ,介绍了红外光学系统优化设计的方法 ,给出了设计结果 ,并与国内同类地球模拟器的光学特性进行比较 ,说明准直式地球模拟器光学系统设计是成功的。     

FY—1C卫星的资料处理及应用研究

介绍了FY－1C的轨道特征、对地观测能力、星上数据贮存能力和数据传输能力等，以及卫星仪器特性、光谱波段特征和应用能力。最后给出了卫星资料的应用情况。     

引射冷却系统设计与数值模拟

采用复合可压流法和考虑粘性影响的一维流法设计了满足最大次流流量的引射喷管冷却结构,并采用Delphi语言开发了具有友好人机界面的设计应用软件,对引射喷管抽吸特性规律进行了研究,利用Fluent商用软件进行了设计引射喷管结构的数值模拟,验证了计算方法的有效性.     

太阳矢量在行星际探测器姿态估计中的应用研究

在基于矢量观测的行星际探测器姿态确定中,参考矢量的几何关系是影响姿态估计精度的一个重要因素。针对这一问题,本文提出了一种利用太阳矢量来提高探测器姿态估计精度的最优算法。该方法在引入太阳矢量的基础上,将星敏感器测得的姿态四元数转化为两个互相垂直的参考矢量,并根据敏感器的测量精度计算相应的规范化权值系数;结合姿态四元数估计算法,给出最小二乘意义下的探测器最优姿态估计。最后,以深度撞击任务的实际飞行数据对本文所提算法进行验证。仿真结果表明,引入太阳矢量后的三轴姿态角估计误差小于150μrad,完全满足深度撞击任务的要求。     

Effects of in-track maneuver on Sun illumination conditions of near-circular low Earth orbits

By developing approximate analytical models considering the J₂ perturbation, the effects of an in-track maneuver on the orbital Sun illumination conditions of near-circular low Earth orbits are analyzed. First, two approximate models for the variations in orbital sunshine angles are developed, one for variations at a given time and the other for variations at a given argument of latitude. Next, two approximate models for variations in orbital arc in Earth shadow are developed, one considers the small eccentricity and the other uses the zero eccentricity. Finally, the developed approximate models are applied to analyzing the Sun illumination conditions of a typical in-track maneuver mission on a near-circular low Earth orbit. From the results obtained, three major conclusions can be drawn. First, the variations in orbital sunshine angles at a given time may reach tens of degrees when the drifting time reaches hundreds of orbital periods, and the approximate model for that situation cannot effectively approach the numerical results. Second, the variations in orbital sunshine angles for any given argument of latitude are only a couple of degrees even when the drifting time reaches 500 orbital periods, and the approximation model developed can effectively approach the numerical results. Third, for variations in orbital arc in Earth shadow, the approximate model considering the small eccentricity has simple expressions and can effectively approach the numerical results; in contrast, the approximate model using the zero eccentricity has relatively worse precision.     

基于混杂非对称复合材料的自适应对日定向器

提出并设计了一种基于混杂非对称复合材料层合板的新型自适应对日定向器。该对日定向器采用混杂非对称复合材料层合板作为驱动元件,利用在轨光照条件的变化引起复合材料层合板温度变化,进而使其产生热变形并驱动太阳翼发生偏转。提出的自适应对日定向器结合传统的单自由度对日定向机构,能够实现太阳能帆板的双自由度对日定向。介绍了自适应对日定向器的基本原理,并结合地球静止轨道的光照条件进行了具体设计。利用能量变分原理建立了混杂非对称复合材料的热变形模型,分析其热变形特点,并利用有限元方法对定向器在地球静止轨道上的温度场特性、热变形及对日定向转动角度进行分析。有限元分析结果表明,通过合理设计,自适应对日定向器的转角能够随太阳光入射角变化呈线性变化,定向精度可达±1°。     

FCD1软脆光学镜片的高效研磨加工

针对FCD1软脆光学镜片高效高成品率的精密加工问题,本研究提出了一种使用复合结合剂金刚石丸片的精研加工技术,其金刚石丸片研具采用了金属、树脂和添加剂等复合结合剂。在精研过程中,丸片表层金刚石磨粒对工件的切深一致性避免了工件表面易出现的深划痕,可有效减少后道抛光工序加工时间,从而提高FCD1软脆光学镜片的生产效率和成品率。     

The gas pixel detector as a solar X-ray polarimeter and imager

The Sun is the nearest astrophysical source with a very intense emission in the X-ray band. The study of energetic events, such as solar flares, can help us to understand the behaviour of the magnetic field of our star. There are in the literature numerous studies published about polarization predictions, for a wide range of solar flares models involving the emission from thermal and/or non-thermal processes, but observations in the X-ray band have never been exhaustive.The gas pixel detector (GPD) was designed to achieve X-ray polarimetric measurements as well as X-ray images for far astrophysical sources. Here we present the possibility to employ this instrument for the observation of our Sun in the X-ray band.